Dynamical variables and evolution of the universe

DOI10.1142/S0218271817500298zbMath1358.83112MaRDI QIDQ2971403

Z. Yousaf, M. Zaeem Ul Haq Bhatti

Publication date: 5 April 2017

Published in: International Journal of Modern Physics D (Search for Journal in Brave)

zbMATH Keywords

\(f(R)\) gravityrelativistic dissipative fluidsstructure scalars

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Quantum hydrodynamics and relativistic hydrodynamics (76Y05)

Related Items (13)

Role of modified scalar variables in the modeling of spherical fluids ⋮ Shear and expansion evolution for dissipative fluids ⋮ Quasi static evolution of compact objects in modified gravity ⋮ Energy conditions in higher derivative f(R,□R,T) gravity ⋮ Some anisotropic planar stellar models ⋮ Influence of modification of gravity on spherical wormhole models ⋮ Stability of anisotropic stellar filaments ⋮ Charged traversable wormholes in f(R) gravity ⋮ Tolman mass of spherical fluids with electromagnetic field ⋮ Structure scalars with charged dissipative systems in \(f(G, T)\) gravity ⋮ Energy conditions in modified \(f(G)\) gravity ⋮ Role of f(G,T) gravity on the evolution of relativistic stars ⋮ Energy content of a collapsing sphere with f(R) gravity

Cites Work

• Modified gravity with ln \(R\) terms and cosmic acceleration
• An exponential \(F(R)\) dark energy model
• The cosmology in f(R,τ) gravity without dark energy
• POWER-LAWS f(R) THEORIES ARE COSMOLOGICALLY UNACCEPTABLE
• Effects of some physical factors on the stability of collapsing stars
• Republication of: Relativistic cosmology

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